Inhomogeneity of the actual value of the vacuum energy density is considered
in a black hole background. We examine the back-reaction of a Schwarzschild
black hole to the highly inhomogeneous vacuum density, and argue the
fluctuations lead to deviations from general relativity in the near-horizon
region. In particular, we found that vacuum fluctuations onto the horizon
trigger adiabatic release of quantum information, while vacuum fluctuations in
the vicinity of the horizon produce potentially observable metric fluctuations
of order the Schwarzschild radius. Consequently, we propose a form of strong
nonviolent nonlocality in which we simultaneously get nonlocal release of
quantum information, and observable metric fluctuations.